SDO HMI 2014-03-29 10:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.33 | 31.37 | 1.80 | 16.90 | 3.79 | 138.71 | 20.68 | 296.41 | 0.3947 | 195.9 | 233.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.88 | 0.00 | 0.49 | 5.30 | 142.40 | 24.37 | 295.64 | 0.4577 | -594.0 | -456.0 | |
| 0.00 | 1.58 | 0.00 | 0.87 | 3.46 | 142.04 | 24.01 | 292.22 | 0.4405 | -827.0 | -696.1 | |
| 1.49 | 2.80 | 0.82 | 1.55 | 4.76 | 141.98 | 23.95 | 294.96 | 0.4482 | -991.8 | -812.3 | |
| 0.00 | 1.40 | 0.00 | 0.78 | 5.13 | 141.90 | 23.87 | 295.77 | 0.4494 | -842.0 | -690.7 | |
| 0.00 | 2.10 | 0.00 | 1.16 | 4.97 | 141.27 | 23.24 | 296.09 | 0.4396 | -916.0 | -785.4 | |
| 0.00 | 2.19 | 0.00 | 1.20 | 4.59 | 140.96 | 22.93 | 295.62 | 0.4326 | -679.0 | -659.9 | |
| 0.00 | 1.40 | 0.00 | 0.75 | 2.39 | 138.48 | 20.45 | 293.28 | 0.3817 | 880.0 | 638.6 | |
| 0.00 | 2.28 | 0.00 | 1.21 | 2.44 | 137.33 | 19.31 | 294.69 | 0.3651 | 861.0 | 686.5 | |
| 0.00 | 1.58 | 0.00 | 0.84 | 3.65 | 137.36 | 19.33 | 297.60 | 0.3744 | 766.0 | 633.4 | |
| 0.00 | 1.31 | 0.00 | 0.70 | 3.99 | 137.37 | 19.34 | 298.38 | 0.3771 | 698.0 | 626.8 | |
| 0.00 | 0.70 | 0.00 | 0.37 | 4.11 | 137.27 | 19.25 | 298.78 | 0.3767 | 872.0 | 771.1 | |
| 1.84 | 7.27 | 0.98 | 3.86 | 2.70 | 137.02 | 18.99 | 295.71 | 0.3624 | 1077.2 | 910.3 | |
| 0.00 | 2.72 | 0.00 | 1.45 | 3.64 | 137.04 | 19.01 | 297.98 | 0.3698 | 913.0 | 685.3 | |
| 0.00 | 1.23 | 0.00 | 0.65 | 4.79 | 136.09 | 18.06 | 302.01 | 0.3659 | 757.0 | 598.8 | |
| 0.00 | 1.93 | 0.00 | 1.02 | 4.79 | 135.87 | 17.84 | 302.32 | 0.3628 | 768.0 | 594.4 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
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| Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
| Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
| B | - Heliographic latitude B; positive: North, negative: South | |
| L | - Heliographic longitude L | |
| LCM | - Longitudinal distance from the Sun's central meridian | |
| Pos. angle | - Position angle | |
| r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
| MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
| MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. | |